Variable Stars in Canis Minor, November 2004
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Canis Minor is the target of my interest since I purchased a ccd camera.
In the first year of my ccd observing I have had serious difficulties to get
the desired object onto the chip. In Canis Minor I could find Procyon first
and there where no doubts of identity. Most of the other stars are only a few
rotations of the adjustment screws away and may be found in a few minutes.
The ccd camera allows to observe all the faint stars that have been neglected
since their discovery.

The following states of the elements are distinguished:
* elements correct, forecast for 2005 possible
+ elements in doubt, forecast for 2005 possible
- elements probably wrong, no relaiable forecast possible
0 star not yet observed by me

X * GCVS period was alias, corrected by E.Schmidt
Y - 3 maxima observed, no forecast
RS * GCVS period was alias
RT *
RV *
RW * period found
RX * displaced secondary
RY *
SX + based on Rotse and Asas data
SY - 1 maximum found but period too inaccurate
TT *
TU *
TW + based on minimum observed by M.Zejda
TX *
TY *
TZ - 1 minimum found, Rotse and Asas not conclusive
UY +
UZ *
XZ *
YY *
AA *
AB + minimum found
AC *
AD 0
AG *
AK *
AL *
AM *
AN *
AO *
AP *
AR - period found, but probably wrong
AS + period found, may be alias
AT - faint, little observed until now
AU 0 faint
AV * displaced secondary minimum?
AY -
BB * type probably EW
BF *
BH *
BI 0 small amplitude (DSCT)
BL * was NVS 3570, period found
BU + period based on Asas data
BV 0 Hipparcos, bright, small amplitude
BX 0 was NSV 3438
BY - was NSV 3624, 3 minima found, period unknown
BZ 0 discovered by K.Bernhard
CW 0 IBVS 4844
NSV 3521 + period found by j.Vanderbroere contradicted by Rotse data
NSV 3637 - no minimum found yet
G0766.1248 0 BrhV040 discovered by K.Bernhard
G0763.0572 0 BrhV103 discovered by K.Bernhard
G0181.1180 0 discovered by Asas
G0181.2426 0 discovered by Asas